Finite Amplitude Compression Waves in a Collision Free Plasma
Finite Amplitude Compression Waves in a Collision Free Plasma
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In our eReader you can find the full English version of the book. Read Finite Amplitude Compression Waves in a Collision Free Plasma Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book Finite Amplitude Compression Waves in a Collision Free Plasma
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For an initially cold plasma, then, these results depend on three parameters as shown in Figure 10: the initial field orientation 9, the mass ratio e, and the Alfven Mach number M, (or the final strength of the imposed field).
In the two limits (i) 9 = 7r/2, 2(1 + sin 0), i. E. After breaking occurs. Then the time dependent solution rapidly converges to this as was shown in the earlier paper [26] on the transverse case. Even for smaller Mach numbers the time dependent solutions can be quite ac...curately predicted; the amplitude of the wave front and the oscillations behind it can be obtained from the soli- tary wave solution (3-29); and the period of the oscillations is given to within about 25^ by the linear analysis at the fast shock singularity (3-28). In particular, to lowest order in 2 2 2 m = M. - 1, the peak magnetic field is B^ = sin + m cosec 9 and the period 27r/m. But note that these oscillations do not strictly correspond to any steady flow oscillations for the entropy is still zero in these cases.
What to read after Finite Amplitude Compression Waves in a Collision Free Plasma?
You can find similar books in the "Read Also" column, or choose other free books by K W Morton to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
For an initially cold plasma, then, these results depend on three parameters as shown in Figure 10: the initial field orientation 9, the mass ratio e, and the Alfven Mach number M, (or the final strength of the imposed field).
In the two limits (i) 9 = 7r/2, 2(1 + sin 0), i. E. After breaking occurs. Then the time dependent solution rapidly converges to this as was shown in the earlier paper [26] on the transverse case. Even for smaller Mach numbers the time dependent solutions can be quite ac...curately predicted; the amplitude of the wave front and the oscillations behind it can be obtained from the soli- tary wave solution (3-29); and the period of the oscillations is given to within about 25^ by the linear analysis at the fast shock singularity (3-28). In particular, to lowest order in 2 2 2 m = M. - 1, the peak magnetic field is B^ = sin + m cosec 9 and the period 27r/m. But note that these oscillations do not strictly correspond to any steady flow oscillations for the entropy is still zero in these cases.
What to read after Finite Amplitude Compression Waves in a Collision Free Plasma?
You can find similar books in the "Read Also" column, or choose other free books by K W Morton to read onlineMoreLess
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